The available data on nuclear fusion cross sections important to energy generation in the
Sun and other hydrogen-burning stars and to solar neutrino production are summarized and …

In this review, we discuss the present status of three indirect techniques that are used to
determine reaction rates for stellar burning processes, asymptotic normalization coefficients …

An update of the NACRE compilation [3] is presented. This new compilation, referred to as
NACRE II, reports thermonuclear reaction rates for 34 charged-particle induced, two-body …

The Trojan Horse Method (THM) represents an indirect path to determine the bare nucleus
astrophysical S-factor for reactions among charged particles at astrophysical energies. This …

The B 11 (p, α 0) Be 8 reaction was studied from 1 MeV down to astrophysical energies by
means of the Trojan-horse method applied to the H 2 (B 11, α o Be 8) n three-body reaction …

The cross sections of the 2 H (d, p) 3 H and 2 H (d, n) 3 He reactions have been measured
via the Trojan Horse method applied to the quasi-free 2 H (3 He, p 3 H) 1 H and 2 H (3 He, n …

The study of energy production and nucleosynthesis in stars requires an increasingly
precise knowledge of the nuclear reaction rates at the energies of interest. To overcome the …

The quest to comprehend how nuclear processes influence astrophysical phenomena is
driving experimental and theoretical research programs worldwide. One of the main goals in …

In this review, we discuss the new recent results of the Trojan Horse Method that is used to
determine reaction rates for nuclear processes in several astrophysical scenarios. The …

The Trojan Horse Method represents an indirect approach to investigate reactions of
astrophysical relevance at the energies of interest, free of Coulomb suppression and …